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Solar noise storms coordinated observations: May 16–24, 1981

Summary of results of a cooperative study

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Abstract

We present the main results obtained from the coordinated observations of solar radio noise storms organized by C.E.S.R.A. in May 1981. They concern the structure and polarization of radio sources, and the relation with the photospheric magnetic field. A model of coronal magnetic field, accounting for the observations, is briefly discussed.

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References

  • Elgarøy, O.: 1977, Solar Noise Storms, Pergamon Press, New York.

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  • Elgarøy, O., Mercier, C., Tlamicha, A., and Zlobec, P. (eds.): 1983, Proceedings of the 4th CESRA Meeting, Inst. of Theoretical Astrophysics, Blindern, Oslo.

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  • Kerdraon, A. and Mercier, C.: 1982, in A. O. Benz and P. Zlobec (eds.), Proceedings of the 4th CESRA Workshop on Solar Noise Storms, p. 27.

  • Sheridan, K. V.: 1982, in A. O. Benz and P. Zlobec (eds.), Proceedings of the 4th CESRA Workshop on Solar Noise Storms, p. 17.

  • Tlamicha, A.: 1982, in A. O. Benz and P. Zlobec (eds.), Proceedings of the 4th CESRA Workshop on Solar Noise Storms, p. 52.

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Authors and Affiliations

  1. Observatoire de Meudon, DASOP and LA 324, 92195, Meudon Principal, CEDEX, France

    C. Mercier

  2. Institute of Theoretical Astrophysics, University of Oslo, Blindern, Norway

    Ø. Elgarøy

  3. Astronomical Observatory, Ondřejov, Czechoslovakia

    A. Tlamicha

  4. Trieste Astronomical Observatory, Italy

    P. Zlobec

Authors
  1. C. Mercier
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  2. Ø. Elgarøy
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  3. A. Tlamicha
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  4. P. Zlobec
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Mercier, C., Elgarøy, Ø., Tlamicha, A. et al. Solar noise storms coordinated observations: May 16–24, 1981. Sol Phys 92, 375–381 (1984). https://doi.org/10.1007/BF00157259

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  • DOI: https://doi.org/10.1007/BF00157259

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